Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Farah, Amanda M"'
Autor:
Kunnumkai, Keerthi, Palmese, Antonella, Farah, Amanda M, Bulla, Mattia, Dietrich, Tim, Pang, Peter T H, Anand, Shreya, Andreoni, Igor, Cabrera, Tomas, Connor, Brendan O
With GW170817 being the only multimessenger gravitational wave (GW) event with an associated kilonova (KN) detected so far, there exists a pressing need for realistic estimation of the GW localization uncertainties and rates, as well as optimization
Externí odkaz:
http://arxiv.org/abs/2411.13673
Autor:
Kunnumkai, Keerthi, Palmese, Antonella, Bulla, Mattia, Dietrich, Tim, Farah, Amanda M., Pang, Peter T. H.
The detection of the gravitational-wave event GW230529, presumably a neutron star-black hole (NSBH) merger, by the LIGO-Virgo-KAGRA (LVK) Collaboration is an exciting discovery for multimessenger astronomy. The black hole (BH) has a high probability
Externí odkaz:
http://arxiv.org/abs/2409.10651
Autor:
Janquart, Justin, Keitel, David, Lo, Rico K. L., Chan, Juno C. L., Ezquiaga, Jose Marìa, Hannuksela, Otto A., Li, Alvin K. Y., More, Anupreeta, Phurailatpam, Hemantakumar, Singh, Neha, Uronen, Laura E., Wright, Mick, Adhikari, Naresh, Biscoveanu, Sylvia, Bulik, Tomasz, Farah, Amanda M., Heffernan, Anna, Joshi, Prathamesh, Juste, Vincent, Kedia, Atul, Nichols, Shania A., Pratten, Geraint, Rawcliffe, C., Roy, Soumen, Sänger, Elise M., Tong, Hui, Trevor, M., Vujeva, Luka, Zevin, Michael
On the 29th of May 2023, the LIGO-Virgo-KAGRA Collaboration observed a compact binary coalescence event consistent with a neutron star-black hole merger, though the heavier object of mass 2.5-4.5 $M_\odot$ would fall into the purported lower mass gap
Externí odkaz:
http://arxiv.org/abs/2409.07298
Autor:
Farah, Amanda M., Callister, Thomas A., Ezquiaga, Jose María, Zevin, Michael, Holz, Daniel E.
Gravitational waves (GWs) from merging compact objects encode direct information about the luminosity distance to the binary. When paired with a redshift measurement, this enables standard-siren cosmology: a Hubble diagram can be constructed to direc
Externí odkaz:
http://arxiv.org/abs/2404.02210
When modeling the population of merging binary black holes, analyses have generally focused on characterizing the distribution of primary (i.e. more massive) black holes in the binary, while simplistic prescriptions are used for the distribution of s
Externí odkaz:
http://arxiv.org/abs/2308.05102
Autor:
Kiendrebeogo, R. Weizmann, Farah, Amanda M., Foley, Emily M., Gray, Abigail, Kunert, Nina, Puecher, Anna, Toivonen, Andrew, VandenBerg, R. Oliver, Anand, Shreya, Ahumada, Tomás, Karambelkar, Viraj, Coughlin, Michael W., Dietrich, Tim, Kam, S. Zacharie, Pang, Peter T. H., Singer, Leo P., Sravan, Niharika
Publikováno v:
The Astrophysical Journal , 2023, 958, 158
An advanced LIGO and Virgo's third observing run brought another binary neutron star merger (BNS) and the first neutron-star black hole mergers. While no confirmed kilonovae were identified in conjunction with any of these events, continued improveme
Externí odkaz:
http://arxiv.org/abs/2306.09234
Autor:
Farah, Amanda M., Edelman, Bruce, Zevin, Michael, Fishbach, Maya, Ezquiaga, Jose María, Farr, Ben, Holz, Daniel E.
Several features in the mass spectrum of merging binary black holes (BBHs) have been identified using data from the Third Gravitational Wave Transient Catalog (GWTC-3). These features are of particular interest as they may encode the uncertain mechan
Externí odkaz:
http://arxiv.org/abs/2301.00834
We search for features in the mass distribution of detected compact binary coalescences which signify the transition between neutron stars and black holes. We analyze all gravitational wave detections by LIGO-Virgo-KAGRA made through the end of the f
Externí odkaz:
http://arxiv.org/abs/2111.03498
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.